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Ultraluminous X-ray sources
We review observations of ultraluminous X-ray sources (ULXs). X-ray spectroscopic and
timing studies of ULXs suggest a new accretion state distinct from those seen in Galactic …
timing studies of ULXs suggest a new accretion state distinct from those seen in Galactic …
A CEERS discovery of an accreting supermassive black hole 570 Myr after the Big Bang: identifying a progenitor of massive z> 6 quasars
We report the discovery of an accreting supermassive black hole at z= 8.679. This galaxy,
denoted here as CEERS_1019, was previously discovered as a Lyα-break galaxy by …
denoted here as CEERS_1019, was previously discovered as a Lyα-break galaxy by …
Formation of the first stars and black holes
We review the current status of knowledge concerning the early phases of star formation
during cosmic dawn. This includes the first generations of stars forming in the lowest mass …
during cosmic dawn. This includes the first generations of stars forming in the lowest mass …
Radiation backgrounds at cosmic dawn: X-rays from compact binaries
We compute the expected X-ray diffuse background and radiative feedback on the
intergalactic medium (IGM) from X-ray binaries prior to and during the epoch of reionization …
intergalactic medium (IGM) from X-ray binaries prior to and during the epoch of reionization …
Building up the Population III initial mass function from cosmological initial conditions
A Stacy, V Bromm, AT Lee - Monthly Notices of the Royal …, 2016 - academic.oup.com
We simulate the growth of a Population III stellar system, starting from cosmological initial
conditions at z= 100. We follow the formation of a minihalo and the subsequent collapse of …
conditions at z= 100. We follow the formation of a minihalo and the subsequent collapse of …
Galaxy properties and UV escape fractions during the epoch of reionization: results from the renaissance simulations
Cosmic reionization is thought to be primarily fueled by the first generations of galaxies. We
examine their stellar and gaseous properties, focusing on the star formation rates and the …
examine their stellar and gaseous properties, focusing on the star formation rates and the …
Impact of the cosmic background radiation on the initial mass function of metal-poor stars
S Chon, H Ono, K Omukai… - Monthly Notices of the …, 2022 - academic.oup.com
We study star cluster formation at low metallicities of Z/Z⊙= 10− 4–10− 1 using three-
dimensional hydrodynamics simulations. Particular emphasis is put on how the stellar mass …
dimensional hydrodynamics simulations. Particular emphasis is put on how the stellar mass …
The birth of a massive first-star binary
We study the formation of massive Population III binary stars using a newly developed
radiation hydrodynamics code with the adaptive mesh refinement and adaptive ray-tracing …
radiation hydrodynamics code with the adaptive mesh refinement and adaptive ray-tracing …
thesan-hr: galaxies in the Epoch of Reionization in warm dark matter, fuzzy dark matter, and interacting dark matter
Using high-resolution cosmological radiation-hydrodynamic (RHD) simulations (thesan-hr),
we explore the impact of alternative dark matter (altDM) models on galaxies during the …
we explore the impact of alternative dark matter (altDM) models on galaxies during the …
Trap** of H ii regions in Population III star formation
O Jaura, SCO Glover, KMJ Wollenberg… - Monthly Notices of …, 2022 - academic.oup.com
Radiative feedback from massive Population III (Pop III) stars in the form of ionizing and
photodissociating photons is widely believed to play a central role in shutting off accretion …
photodissociating photons is widely believed to play a central role in shutting off accretion …